Inspiral into Gargantua
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Publication:2820651
DOI10.1088/0264-9381/33/15/155002zbMath1346.83026arXiv1603.01221OpenAlexW2291192580MaRDI QIDQ2820651
Samuel E. Gralla, Niels Warburton, Scott Alexander Hughes
Publication date: 9 September 2016
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1603.01221
Black holes (83C57) Spinor and twistor methods in general relativity and gravitational theory; Newman-Penrose formalism (83C60) Galactic and stellar structure (85A15) Gravitational waves (83C35)
Related Items (14)
Gravitational waves from plunges into Gargantua ⋮ Planar black holes as a route to understanding the weak gravity conjecture ⋮ Thermal ringdown of a Kerr black hole: overtone excitation, Fermi-Dirac statistics and greybody factor ⋮ Whirling orbits around twirling black holes from conformal symmetry ⋮ Semi-local quantum criticality and the instability of extremal planar horizons ⋮ Late-time asymptotics for the wave equation on extremal Reissner-Nordström backgrounds ⋮ Near-extremal black holes at late times, backreacted ⋮ Gravitational perturbations from NHEK to Kerr ⋮ Spin and quadrupole couplings for high spin equatorial intermediate mass-ratio coalescences ⋮ Polarization whorls from M87* at the event horizon telescope ⋮ Particle motion near high-spin black holes ⋮ Transition from inspiral to plunge into a highly spinning black hole ⋮ Force-free magnetosphere attractors for near-horizon extreme and near-extreme limits of Kerr black hole ⋮ The Kerr/CFT correspondence and its extensions
Cites Work
- The large \(N\) limit of superconformal field theories and supergravity
- Gravitational collapse: The role of general relativity
- Microscopic origin of the Bekenstein-Hawking entropy
- Fast plunges into Kerr black holes
- Where is the extremal Kerr ISCO?
- Quasinormal modes of black holes and black branes
- The overlap of numerical relativity, perturbation theory and post-Newtonian theory in the binary black hole problem
- The spin of supermassive black holes
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